Atmospheric Background Measurement in the 300-400 nm Band with a Balloon Borne Experiment During a Nocturnal Flight (Articolo in rivista)

Type
Label
  • Atmospheric Background Measurement in the 300-400 nm Band with a Balloon Borne Experiment During a Nocturnal Flight (Articolo in rivista) (literal)
Anno
  • 2001-01-01T00:00:00+01:00 (literal)
Alternative label
  • 1)La Rosa, Giovanni; 2) Agnetta, Gaetano; 3) Biondo, Benedetto; 4) Catalano, Osvaldo; 5) Celi, Filippo; 6) Di Raffaele, Renato; 7)Giarrusso, Salvatore; 8) Mangano, Angelo; 9) Russo, Francesco; 10) Linsley, John; 11) Lo Bue, Angelo (2001)
    Atmospheric Background Measurement in the 300-400 nm Band with a Balloon Borne Experiment During a Nocturnal Flight
    in Astrophysics and space science
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • 1)La Rosa, Giovanni; 2) Agnetta, Gaetano; 3) Biondo, Benedetto; 4) Catalano, Osvaldo; 5) Celi, Filippo; 6) Di Raffaele, Renato; 7)Giarrusso, Salvatore; 8) Mangano, Angelo; 9) Russo, Francesco; 10) Linsley, John; 11) Lo Bue, Angelo (literal)
Pagina inizio
  • 219 (literal)
Pagina fine
  • 226 (literal)
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  • Times cited= 0 Impact Factor= 0.383 (literal)
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  • 276 (literal)
Rivista
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  • Misura del Background notturno UV in assenza di Luna con un rivelatore trasportato da pallone stratosferico in un volo transmediterraneo. La misura è importante per l’osservazione di Raggi Cosmici di estrema energia attraverso l’osservazione della fluorescenza prodotta in Atmosfera dagli Sciami Estesi. (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1-9)IFCAI, Consiglio Nazionale delle Ricerche, Palermo, Italy), 10)PANDA, University of New Mexico, Albuquerque NM, U.S.A.), 11)Electronic Engineering Department, University of Palermo, Italy) (literal)
Titolo
  • Atmospheric Background Measurement in the 300-400 nm Band with a Balloon Borne Experiment During a Nocturnal Flight (literal)
Abstract
  • The balloon borne experiment, named BABY (BAckground BYpass) belongs to a wider program, AIRWATCH-OWL, intended for the observation of high energy Cosmic Rays from space, detecting the faint UV fluorescence light emitted by the atmospheric Nitrogen as final result of a complex hadronic cascade. In this framework, one of the fundamental information concern the knowledge of the background level. This is one of the main parameters that contribute to the sensitivity of any kind of instrument. The apparatus used for the BABY experiment was designed and completely built at the IFCAI-CNR in Palermo. The instrument is composed by two filtered and collimated photomultipliers (PMT) that detect the UV light in the 300-400 nm wavelength. We report a brief description of the design of the detector and the results coming from a preliminary analysis of the data taken during a nocturnal over-sea observation. (literal)
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